OBJECT                         = DATA_SET
DATA_SET_ID                    = "ICE-C-SWPLAS-3-RDR-GIACOBIN-ZIN-V1.0"

OBJECT                         = DATA_SET_INFORMATION 
DATA_SET_NAME                  = "ICE SOLAR WIND PLASMA ELECTRON ANALYSER DATA 
V1.0"

DATA_SET_COLLECTION_MEMBER_FLG = Y
START_TIME                     = 1985-09-10T00:00:16.800Z
STOP_TIME                      = 1985-09-14T20:46:53.200Z
DATA_SET_RELEASE_DATE          = UNK
PRODUCER_FULL_NAME             = "INTERNATIONAL HALLEY WATCH"
DETAILED_CATALOG_FLAG          = N
DATA_SET_DESC                  = "

\v
  Data Set Overview
  =================
\v

 These data were obtained from the LANL plasma experiment on ICE (Principal
 Investigator: S.J. Bame; data provided by J.T. Gosling, with assistance                                                          
 from K. Sofaly and S. Kedge). The instrument measures the 2-D electron                                                           
 distribution function in one spacecraft rotation (3 s) once every 24 s, by                                                       
 obtaining 16 evenly spaced energy spectra, each with 15 contiguous levels                                                        
 covering the energy range 8.5 eV to 1140 eV.   From these 2-D distributions                                                      
 the density, velocity, and temperature of the electrons are then derived.                                                        
 A 2-D temperature matrix is calculated which is subsequently diagonalized.                                                       
 Then nominally the maximum temperature corresponds to the parallel                                                               
 temperature and the minimum temperature corresponds to the perpendicular                                                         
 temperature. This is done independently of the magnetic field measurements;                                                      
 however, the direction of maximum temperature determined in this manner is                                                       
 usually found to be within 15 degrees of the magnetic field direction                                                            
 inferred from the magnetometer measurements.   The time resolution is 24 sec
 from the start of Day 253 (September 10) until Day 255 (September 12),
 18:38. At that time the bit rate dropped from 1024 to 512 bps, and the                                                           
 nominal time resolution went to 48 sec.
                                                                                                                                  
"

CONFIDENCE_LEVEL_NOTE          = "

\v
  Confidence Level Overview
  =========================
\v

         N/A"
END_OBJECT                     = DATA_SET_INFORMATION

OBJECT                         = DATA_SET_TARGET
TARGET_NAME                    = "GIACOBINI-ZINNER"
END_OBJECT                     = DATA_SET_TARGET                    

OBJECT                         = DATA_SET_HOST
INSTRUMENT_HOST_ID             = ICE
INSTRUMENT_ID                  = SWPLAS
END_OBJECT = DATA_SET_HOST

OBJECT                         = DATA_SET_REFERENCE_INFORMATION
REFERENCE_KEY_ID               = "ESA-SP1066"
END_OBJECT                     = DATA_SET_REFERENCE_INFORMATION

END_OBJECT       = DATA_SET
END